Abstract The Interior exploration using Seismic Investigations, Geodesy, and Heat Transport
(InSight) Mission will focus on Mars' interior structure and evolution. The basic structure of …

Clues to a planet's geologic history are contained in its interior structure, particularly its core.
We detected reflections of seismic waves from the core-mantle boundary of Mars using …

The first samples collected by the Mars 2020 mission represent units exposed on the Jezero
Crater floor, from the potentially oldest Séítah formation outcrops to the potentially youngest …

We invert the Martian tidal response and mean mass and moment of inertia for chemical
composition, thermal state, and interior structure. The inversion combines phase equilibrium …

The present‐day thermal state, interior structure, composition, and rheology of Mars can be
constrained by comparing the results of thermal history calculations with geophysical …

We employ laboratory‐based grain size‐and temperature‐sensitive rheological models to
describe the viscoelastic behavior and tidal response of terrestrial bodies with focus on …

We investigate the coupled evolution of the atmosphere and mantle on Venus. Here we
focus on mechanisms that deplete or replenish the atmosphere: atmospheric escape to …

Water has been stored in the Martian mantle since its formation, primarily in nominally
anhydrous minerals. The short-lived early hydrosphere and intermittently flowing water on …

Studies of rocks in Gale Crater and clasts within the Martian meteorite breccia Northwest
Africa (NWA) 7034 (and paired stones) have expanded our knowledge of the diversity of …

A giant impact is commonly thought to explain the dramatic contrast in elevation and crustal
thickness between the two hemispheres of Mars known as the “Martian Dichotomy”. Initially …